activity
20002006
most citedMSSM flat direction inflation: slow roll, stability, fine tunning and reheating

235 citations · 1.1k across the 18 of their papers we have counts for

collaborators

18 papers

hep-ph2006★ 5 cited

Sub-eV Hubble scale inflation within gauge mediated supersymmetry breaking

Rouzbeh Allahverdi, Asko Jokinen, Anupam Mazumdar

Minimal Supersymmetric Standard Model with gauge mediated supersymmetry breaking has all the necessary ingredients for a successful sub-eV Hubble scale inflation $H_{\rm inf} \sim…

hep-ph2006★ 235 cited

MSSM flat direction inflation: slow roll, stability, fine tunning and reheating

Rouzbeh Allahverdi, Kari Enqvist, Juan Garcia-Bellido +2

We consider low scale slow roll inflation driven by the gauge invariant flat directions {\bf udd} and {\bf LLe} of the Minimally Supersymmetric Standard Model at the vicinity of a…

hep-ph2006★ 41 cited

Identifying the curvaton within MSSM

Rouzbeh Allahverdi, Kari Enqvist, Asko Jokinen +1

We consider inflaton couplings to MSSM flat directions and the thermalization of the inflaton decay products, taking into account gauge symmetry breaking due to flat direction cond…

astro-ph2006★ 80 cited

Very Large Primordial Non-Gaussianity from multi-field: Application to Massless Preheating

Asko Jokinen, Anupam Mazumdar

In this paper we derive a generic expression, which is valid for scales larger than Hubble radius and contains only the local terms, for the second order curvature perturbations fo…

hep-ph2005★ 7 cited

Supermassive gravitinos, dark matter, leptogenesis and flat direction baryogenesis

Rouzbeh Allahverdi, Steen Hannestad, Asko Jokinen +2

In general the gravitino mass and/or the soft supersymmetry breaking masses in the observable sector can be much larger than the TeV scale. Depending on the relation between the ma…

hep-th2005★ 29 cited

Cosmological constraints on string scale and coupling arising from tachyonic instability

Kari Enqvist, Asko Jokinen, Anupam Mazumdar +2

We demonstrate that string motivated inflation ending via tachyonic instability leaves a detectable imprint on the cosmic microwave background (CMB) radiation by virtue of the exci…